Mentz114 said:
I must disagree, because you're not measuring curvature. You're fitting observations to a theory that uses curvature to model the effects of gravity. Sure, we can measure the curvature of a physical thing like a football or a piece of string. But what are you measuring the curvature of when it's 'spacetime' ?
Your comments led me to ponder the difference between spatial curvature and spacetime curvature and I came up with this series of scenarios for discussion.
First a list of the terms I use in the discussion:
(1) Optical flatness.
A surface is optically flat if when any two spatially separated points on the surface are connected by a laser beam, then a point mid way along the laser beam will be on the surface. If the surface midpoint is below the light beam, then the surface will be said to have positive optical curvature.
(2) Gravitational flatness.
A surface is gravitationally flat if objects that are free to move stay where they are. If objects all tend to roll towards a common point then the surface will be said to be have positive gravitational curvature and if all objects tend to roll away from each other then the surface will be said to have negative gravitational curvature. Saddle points on a surface will have a mixture of positive and negative gravitational curvature that is directionally dependent but I don't think this is a major worry, because such a spatial saddle point will presumably fail all other flatness tests. I think almost by definition, spatially separated clocks on a gravitationally flat surface will run at the same rate.
(3)Euclidean flatness.
A surface is Euclidean flat if the internal angles of any traiangle on the surface add up to 180 degrees and if the ratio of the circumference to the radius of any circle on the surface is 2Pi, measured from a point at the centre of the circle but also on the surface. If the circle ratio is less than 2Pi or the triangle angles add up to more than 180 degrees, then the surface will be said to have positive Euclidean curvature.
(4) Spatial flatness.
For this definition I define a hypothetical "rigid" plane that is constructed out of Unobtainium, far away from any gravitational sources. At the time of construction the rigid plane is designed and tested to have optical and Euclidean flatness and is sufficiently rigid to resist being physically bent by gravitational forces. This rigid plane is meant to be a "spatial flatness ruler" that can be transported to where we want to measure flatness.
Now the question is which of the above definitions most closely describes spacetime curvature?
Here are some scenarios for possible discussion.
Consider a neutron star that conveniently has a radius equal to its photon orbit radius. The surface of this star would be optically and gravitationally flat and "look" flat to an observer standing on the surface of the star. It would not be spatially flat when compared to the rigid plane and it will have considerable positive Euclidean curvature.
Now imagine the rigid plane is placed close to this star so that the centre of the plane is closest to the star and the plane is orthogonal to a radial line from the centre of the star. To an observer on this "rigid spatially flat plane" the plane is not optically flat and will appear to an observer near the centre that he is standing at the lowest point of a bowl depression. The rigid spatial flat plane is also not gravitationally flat in this scenario and objects placed on it will tend to roll towards the centre in agreement with the observers optical perception that he is in a bowl. The rigid plane also fails the Euclidean flatness test. The rigid flat plane in this situation has positive optical curvature, positive gravitational curvature and positive Euclidean curvature.
Now consider an object with obvious spatial curvature but insignificant gravitation such as a tennis ball. The surface will not have Euclidean flatness because 3 points on the surface can have internal angles greater than 180 degrees. However, if we poke holes in the ball we can see that the 3 points can be connected by laser beams and although the surface has spatial curvature the 3 points are still embedded in flat space. We can still find a point (inside the ball) that is the centre of a circle passing through the 3 points and the radius to circumference ratio is Euclidean. So, although the ball surface is not flat, points on the surface of the ball can still be considered to be embedded in flat space. Now if we transport our ball to very close to an extreme gravitational source, the points on the ball will fail the Euclidean flatness test and so we might conclude there is something different about about the space the ball is embedded in near an extreme gravitational source. Can we call this difference spacetime curvature?
Now consider widely spaced clocks on the surface of the Earth. They are all at sea level and running at the same rate, so they are on a gravitationally flat surface. They are obviously not on an optically flat surface, because sufficiently far points are over the horizon and we cannot connect 3 clocks in a line using a laser. So the Earth's surface is gravitationally flat but not spatially flat, optically flat or Euclidean flat. Is there any evidence of spacetime curvature here? Let us slice a piece off the Earth that is spatially flat (as measured by our rigid plane) and place 3 clocks on this cut surface. Will we measure slight positive Euclidean curvature on this "flat surface"? I think we will, as well as slight positive gravitational and optical curvature. While in a destructive mood let us cut off another slice using a powerful laser so that the new cut surface is optically flat. This new cut slice is not spatially, gravitationally or Euclidean flat.
After considering the above scenarios, it would seem one operational definition of spacetime flatness is to define an optically flat surface in the region under consideration and then check for Euclidean flatness on that optically flat surface. If the optically flat surface is not Euclidean flat then it seems there is evidence that there is intrinsic spacetime curvature. Euclidean curvature of a surface does not necessarily prove that the spacetime the surface is embedded in is intrinsically curved and optical flatness of a surface by itself does not demonstrate that the surface is embedded in flat spacetime. It seems we need to perform both tests.
So which if any of the above scenarios best illuminates spacetime curvature rather than just space curvature?
Perhaps the answer is "none of the above". I think Dalespam gave a good example of intrinsic spacetime curvature with the example of the changing spatial separation of two free falling observers due to tidal effects. While clocks in an accelerating rocket show Doppler shift with height as in a gravitational field, sequentially dropped objects in the rocket will maintain constant mutual spatial separation, demonstrating that the presence or absence of intrinsic curvature of the background can be detected even in an accelerating rocket. However, is defining tidal effects as intrinsic spacetime curvature just semantics? Newton would have been very aware of tidal separation of falling particles and it never for a moment led him to consider that this was evidence of time and space changing in some mysterious way.
P.S. I am not taking any strong position on anything I say above and I am just kicking some ideas around so that maybe someone can lead me to a clearer understanding in intuitive terms. Some of my definitions of what is positive or negative curvature may contradict already established formal conventions, so corrections are welcome
